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researcher

N. Mirabal

82 papers hereh-index 3910.9k citations156 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author8
  • first author16
  • middle author16
  • last author4

Across the 44 of 82 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE51
  • astro-ph28
  • astro-ph.GA2
  • astro-ph.IM1
same name
  • N. Mirabal — 21 papers, h 5
  • N. Mirabal — 7 papers
  • N. Mirabal — 1 paper, h 8

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002025
most citedFermi Large Area Telescope Fourth Source Catalog

1.4k citations · 6.7k across the 77 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002★ 30 cited

High Resolution Grating Spectroscopy of GRB 020405 with CHANDRA LETGS

N. Mirabal, F. Paerels, J. P. Halpern

We present high-resolution X-ray spectroscopy of GRB 020405 obtained with the Low Energy Transmission Grating Spectrometer (LETGS) on board the Chandra X-ray Observatory starting 1…

astro-ph2002★ 62 cited

Time-Dependent Optical Spectroscopy of GRB 010222: Clues to the GRB Environment

N. Mirabal, J. P. Halpern, S. R. Kulkarni +9

We present sequential optical spectra of the afterglow of GRB 010222 obtained one day apart using the Low Resolution Imaging Spectrometer (LRIS) and the Echellette Spectrograph and…

astro-ph2002

Multiwavelength Searches of Unidentified EGRET Sources

N. Mirabal, J. Halpern, R. Mukherjee +2

3EG J1835+5918 is the brightest of the so-called unidentified EGRET sources at intermediate galactic latitude (l,b)=(89,25). We obtained complete radio, optical, and X-ray coverage…

astro-ph2002★ 149 cited

The 2001 Superoutburst of WZ Sagittae

J. Patterson, G. Masi, M. Richmond +25

We report the results of a worldwide campaign to observe WZ Sagittae during its 2001 superoutburst. After a 23-year slumber at V=15.5, the star rose within 2 days to a peak brightn…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.